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lbaops:lbamar2016:v537a

v537a

Description Resolving Vela pulsars emission region directly via scintellometry
Antennas Pa-At-Ho-Cd-Ti-Ak
Start 64 06:00:00
Stop 64 10:30:00
PI Jean-Pierre Macquart

Setup lba18cm-2p-2IF:

Station Modes Pa At Ho Cd
Channel 1 IFP#1-LO 1634 - 1650 MHz USB RCP
Channel 2 IFP#1-HI 1650 - 1666 MHz USB RCP
Channel 3 IFP#2-LO 1634 - 1650 MHz USB LCP
Channel 4 IFP#2-HI 1650 - 1666 MHz USB LCP
DAS 1 Skyfreq 1650 MHz
Bandwidth 16 MHz
DAS Mode vsop.pro (telescope)
Station Modes Ti
Channel 1 IFP#1-LO 1634 - 1650 MHz USB LCP
Channel 2 IFP#1-HI 1650 - 1666 MHz USB LCP
DAS 1 Skyfreq 1650 MHz
Bandwidth 16 MHz
DAS Mode vsop.pro (telescope)
Station Modes Ak
Channel 1 IFP#1 1618 - 1682 MHz USB RCP
Channel 2 IFP#2 1618 - 1682 MHz USB LCP
DAS 1 Skyfreq 1650 MHz
Bandwidth 64 MHz
DAS Mode 64MHz_[nf].pro (telescope)

Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v537/v537a


Comments:

Pulsar observation: please disable AGC in DAS, continuous noise cal, and PCAL where applicable.

Observing comments for each antenna:

Observing Logs

Weather

Monica log information - EXPERIMENTAL:

lbaops/lbamar2016/v537a.txt · Last modified: 2016/03/03 19:36 by cormac